Fundamentals

1,200 must-knows for NEET & JEE

The core facts every aspirant should own — each a titled nugget with a real-world story, the concept in plain words, and a memory trick. Works even when the internet doesn't.

1,200 fundamentals

PhysicsWork, Energy & Power· Class 11

Work-energy theorem

Brakes do negative work, draining a car's kinetic energy into heat until it stops.

The net work done on a body equals its change in kinetic energy.

W = ΔKE

Memory trick: Net work = change in KE.

PhysicsWork, Energy & Power· Class 11

Potential energy

Water held behind a dam is stored energy waiting to become electricity.

Stored energy of position: gravitational PE = mgh near Earth.

PE = mgh

Memory trick: Height stores energy.

PhysicsWork, Energy & Power· Class 11

Conservation of energy

A pendulum trades height for speed and back, forever (without friction).

Energy can't be created or destroyed, only transformed; total energy stays constant.

Memory trick: Energy changes form, never vanishes.

PhysicsWork, Energy & Power· Class 11

Power

Two lifts reach the top floor; the more powerful one just gets there faster.

Power is the rate of doing work, P = W/t = Fv.

P = W/t = Fv

Memory trick: Same work, faster = more power.

PhysicsWork, Energy & Power· Class 11

Elastic vs inelastic collision

Billiard balls click almost elastically; a crash where cars crumple is inelastic.

Both conserve momentum; only an elastic collision also conserves kinetic energy.

Memory trick: Elastic keeps KE; inelastic loses it to heat.

PhysicsRotational Motion· Class 11

Torque

You push a door at its handle, not near the hinge — more distance, more turn.

Torque τ = force × perpendicular distance is the turning effect of a force.

τ = rF sinθ

Memory trick: Torque = force × lever arm.

PhysicsRotational Motion· Class 11

Moment of inertia

A tightrope walker's long pole spreads mass out, making rotation sluggish and balance easier.

Rotational 'mass' — resistance to angular acceleration; depends on how mass is distributed about the axis.

I = Σmr²

Memory trick: Mass far from axis counts a lot (distance squared).

PhysicsRotational Motion· Class 11

Angular momentum conservation

A skater pulls their arms in, shrinks I, and spins faster — conserving L.

With no external torque, angular momentum L = Iω is conserved.

L = Iω

Memory trick: Pull in → spin faster.

PhysicsRotational Motion· Class 11

Rolling motion energy

A solid cylinder beats a hollow one down a ramp — less energy 'wasted' spinning.

A rolling body has both translational (½mv²) and rotational (½Iω²) kinetic energy.

KE = ½mv² + ½Iω²

Memory trick: Rolling = moving + spinning energy.

PhysicsGravitation· Class 11

Universal gravitation

The same law that drops an apple holds galaxies together.

Every two masses attract with F = Gm₁m₂/r².

F = Gm₁m₂/r²

Memory trick: Inverse-square: double distance, quarter force.

PhysicsGravitation· Class 11

Acceleration due to gravity

You'd weigh slightly less on a mountaintop than at sea level.

g = GM/R² at a planet's surface; it weakens with altitude and depth.

g = GM/R²

Memory trick: g depends on the planet, not on you.

PhysicsGravitation· Class 11

Escape velocity

Rockets must hit ~40,000 km/h to leave Earth for good.

The minimum speed to break free of a planet's gravity; ≈ 11.2 km/s for Earth.

v = √(2GM/R)

Memory trick: Escape = √2 × orbital speed.

PhysicsGravitation· Class 11

Orbital velocity

The ISS orbits at ~7.8 km/s — forever 'falling' around Earth.

Speed needed to stay in a circular orbit, v = √(GM/r).

v = √(GM/r)

Memory trick: Faster orbit = lower altitude.

PhysicsGravitation· Class 11

Kepler's third law

Outer planets crawl; Neptune takes 165 Earth-years for one lap of the Sun.

The square of a planet's orbital period is proportional to the cube of its orbit radius (T² ∝ r³).

T² ∝ r³

Memory trick: Farther planet → much longer year.

PhysicsGravitation· Class 11

Weightlessness in orbit

Gravity in orbit is still ~90% of surface gravity — they're just falling around the Earth.

Astronauts float because they and their spacecraft are in continuous free fall together, not because gravity is absent.

Memory trick: Free fall = apparent weightlessness.

PhysicsMechanical Properties of Fluids· Class 11

Pressure in a fluid

Your ears hurt at the bottom of a swimming pool because water pressure grows with depth.

Pressure increases with depth: P = P₀ + ρgh.

P = P₀ + ρgh

Memory trick: Deeper = higher pressure.

PhysicsMechanical Properties of Fluids· Class 11

Pascal's law

A car hydraulic lift raises tonnes with a gentle push — pressure shared across a big piston.

Pressure applied to an enclosed fluid is transmitted equally in all directions.

Memory trick: Small force, big area → big force.

PhysicsMechanical Properties of Fluids· Class 11

Archimedes' principle

A steel ship floats because its hull displaces enough water to match its weight.

A submerged body feels an upward buoyant force equal to the weight of fluid it displaces.

Memory trick: Buoyancy = weight of fluid pushed aside.

PhysicsMechanical Properties of Fluids· Class 11

Bernoulli's principle

Aeroplane wings lift because air rushes faster over the top, lowering the pressure there.

In a flowing fluid, faster flow means lower pressure.

P + ½ρv² + ρgh = const

Memory trick: Fast flow = low pressure.

PhysicsMechanical Properties of Fluids· Class 11

Surface tension

Water striders walk on ponds and droplets pull into spheres because of surface tension.

The 'skin' on a liquid caused by cohesive forces pulling surface molecules inward.

Memory trick: Liquids minimise their surface.

PhysicsMechanical Properties of Fluids· Class 11

Viscosity

Honey pours slowly and water quickly — honey is far more viscous.

A fluid's internal friction resisting flow.

Memory trick: Thick fluid = high viscosity.

PhysicsMechanical Properties of Solids· Class 11

Hooke's law

Stretch a spring gently and it springs back; pull too far and it stays bent.

Within the elastic limit, stress is proportional to strain.

stress ∝ strain

Memory trick: Small stretch → restoring force ∝ stretch.

PhysicsMechanical Properties of Solids· Class 11

Young's modulus

Steel has a huge Young's modulus — that's why it barely stretches under load.

A measure of a solid's stiffness: stress divided by longitudinal strain.

Y = stress/strain

Memory trick: Higher modulus = stiffer material.

PhysicsOscillations & Waves· Class 11

Simple harmonic motion

A child on a swing, a guitar string, a vibrating atom — all sing the SHM song.

Oscillation where the restoring force is proportional to and opposite the displacement (F = −kx).

F = −kx

Memory trick: Force pulls back ∝ how far you pushed.

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